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Table 1

Programme stars and the behaviour of their old and new radial velocities with respect to the reference orbital solution, as listed in column ‘Ref. orbit’.

HIP SB9 Spectral type Gaia DR3 SB1/2/c Mask N (new) N (old) ⟨O−C⟩ (new) σ(O−C) (new) σ(O−C) (old) Ref. orbit Rem. Old system ∆RV (km s−1)
183 2966 B4III noRV SB1 Bal 8 95 −1.30 1.10 1.71 (1) R CES −0.71 ± 0.79
443 1 K0IIIb brightG SB1 Arc 17 25 −1.24 4.71 1.25 (2) R Lick/Cape/DAO −0.21 ± 0.25
12390 135 F5V SB2 F0 14,13 18,18 0.41,0.92 0.56,1.62 1.02,1.20 (3) R (a)
14124 153 G0IV−V noRV SB2 G2 29,25 57,15 −2.06,−1.14 2.86,3.68 1.10,1.50 (4) R CamCOR −1.17 ± 0.20
14157 2373 K0V noRV SB2 Arc 16,14 31,31 0.36,−0.04 0.53,0.28 0.14,0.31 (5) R KPNO −2.00 ± 0.06
18216 2016 B5V brightG SB1 Bal 19 74 −2.30 16.71 1.30 (6) R CAT-CES −0.39 ± 0.39
22000 270 Am+sgG5 SB2 SB2 F0 16,15 27,10 −0.31,−1.60 3.36,5.12 5.19,2.83 (7) R Mount Wilson −1.15 ± 0.20 (b)
22701 285 F4III Single Bal 6 14 7.28 9.80 9.58 (8)
25912 2798 K1III Acc7 SB1 Arc 6 12 0.36 0.06 0.37 (9) R CORAVEL +0.15 ± 0.41
26563 350 A4V Single Bal 14 12 1.81 12.61 6.56 (8)
28816 380 A1V+M6II noRV SB1 M4 46 55 −0.09 1.06 1.17 (10) R KPNO +0.05 ± 0.16
31205 407 G9.5IIIBa astrom SB1 Arc 8 68 0.51 0.42 0.40 (11) R CORAVEL +0.02 ± 0.05
32426 2884 F8IV-V+B9.5V (c,d) SB2? (c) Arc 9 56 −0.16 0.19 0.86 (12) R CORAVEL +0.01 ± 0.13
32467 2885 G9III SB1/Acc9 SB1 Arc 3 37 −2.01 4.36 0.28 (12) R CORAVEL +0.07 ± 0.06
33168 2622 K1III+B (e) SB1 (e) Arc 2 71 −0.85 0.03 0.47 (13) R CORAVEL −0.85 ± 0.10
34316 2888 K0 nRV<10 SB1 Arc 14 22 −1.36 1.04 0.45 (12) R CORAVEL +0.07 ± 0.11
34935 2577 K3II+B7.5III nRV<10 SBc (d) Arc 2 28 0.07 0.14 0.27 (14) R CORAVEL +0.25 ± 0.17
36419 3095 ApSrCrEu+F/G SB2 F0 2,2 78,78 −1.33,2.05 0.02,0.99 0.75,0.75 (15)
36652 2765 Fm SB1 F0 6 29 0.02 0.19 0.34 (16)
37041 2579 F5 SB1 SB1 F0 7 28 0.56 0.35 0.38 (14) R CORAVEL +0.20 ± 0.08
38217 1553 S3.5/3 Acc7 SB1 Arc 2 14 0.67 0.48 0.38 (17) R CORAVEL +0.14 ± 0.19
39198 2845 G5 astrom SB1 Arc 22 17 0.42 0.72 0.43 (18) R CfA −0.01 ± 0.09
40944 2749 G8III+A3V brightG SB1 Arc 2 22 0.38 0.02 0.28 (19) R CORAVEL +0.36 ± 0.12
42368 2533 G+A1V SBc (d) Arc/Bal 2 100 −1.18 0.12 0.39 (20) R CamCOR −1.06 ± 0.08
43041 2750 K3III+B/A brightG SB1 Arc 2 15 0.11 0.51 0.32 (19) R CORAVEL −0.25 ± 0.16
43099 1708 A5 SB1 Bal 19 135 10.08 4.17 1.90 (21) R CfA −0.16 ± 0.62
45527 564 K2III brightG SB1 Arc 2 61 0.11 7.87 1.45 (22) R Cape +0.03 ± 0.38
50006 1588 K1IIIBa SB1 Arc 3 23 −0.20 0.49 0.44 (17) R CORAVEL +0.47 ± 0.17
50796 2610 K+MV nRV<10 SB1 Arc 17 38 0.31 0.61 0.59 (23) R CfA +0.44 ± 0.10
51533 1564 KIIIBa nRV<10 SB1 Arc 2 24 0.15 0.52 0.39 (17) R CORAVEL +0.91 ± 0.19
53717 1565 G8Ib/IIBa Acc7 SB1 Arc 2 18 0.20 0.39 0.26 (17) R CORAVEL +0.61 ± 0.69
55505A 2449 K4−5 noRV SB1 Arc 23 152 0.18 7.16 1.14 (24) R CfA +0.11 ± 0.19
55505B 2450 K4−5 noRV SB2+vis Arc 8,16 152,152 −3.04,−0.29 10.33,9.54 1.91,3.90 (24) R CfA −0.38 ± 0.01
57341 2751 G8III+A SBc (d) Arc 2 13 0.13 0.10 0.34 (19)
57791 693 K0III astrom SB1 Arc 6 9 0.81 1.19 0.17 (18) R CfA +0.01 ± 0.07
59750 1692 F9VFe−1.7CH−0.7 SB1 Arc 4 39 0.20 0.19 0.44 (21) R CamCOR +0.30 ± 0.11
63742 3198 G5V SB1 Arc 3 42 −1.34 0.18 0.38 (25) R CamCOR +0.31 ± 0.03
69929 809 A0p nRV<10 SB1 F0 2 39 −2.59 2.43 1.12 (26) R Stromlo −1.6 ± 1.0
69974 811 Am noRV SB2 F0 13,13 130,130 1.18,1.20 1.11,0.29 1.14,0.50 (27) R CfA +1.1 ± 0.10
73007 1566 K0IIIBa Acc7 SB1 Arc 2 55 0.47 0.09 0.36 (17) R CORAVEL +1.02 ± 0.24
73182 1475 M1.5V SB2 Arc 8,7 75,10 0.11,0.07 0.13,0.29 0.81,0.92 (28) R ELODIE/Coralie +0.10 ± 0.05
75379 841 F4V nRV<10 SB1 F0 3 42 0.64 0.05 0.08 (29) R DAO +0.49 ± 0.14
75718 1638 G9V+M0V (f) SB2 (g) Arc 3 97,10 0.57 0.07 0.30,2.02 (30)
84402 2851 K1III brightG SB1 Arc 2 8 −1.51 0.70 0.03 (18) R CfA −1.46 ± 0.11
90135 1046 K0III nRV<10 SB1 Arc 12 7 0.34 0.30 0.003 (18) R CfA −1.15 ± 0.04
90692 1063 G5 nRV<10 SB1 Arc 6 67 −0.21 3.23 1.00 (31)
91751 1072 K0.5III astrom SB1 Arc 3 19 −1.76 0.07 0.01 (29) R Kato +31.83 ± 0.02 (h)
92016 1075 F5V nRV<10 SB2 F0 5,2 65,14 −0.56,−0.25 0.48,0.57 1.80,0.66 (32) R KPNO −1.87 ± 0.24
92726 2059 G5 noRV SB1+SB1 Arc 13 28 1.92 6.88 0.48 (33) R Tokovinin COR +0.86 ± 0.21
95066 1144 G8III−IV brightG SB1 Arc 6 51 −0.52 0.97 1.06 (34) R Lick −0.79 ± 0.19
95176 1147 B8p+F2pe noRV SB1 F0 30 −4.84 8.97 (35) R (a)
100738 1239 K3V SB1 Arc 3 93 0.13 0.05 0.15 (36)
104785 2149 G0 Acc9 SB1 Arc 4 19 0.22 0.12 0.47 (37) R DAO +0.60 ± 0.37
110388 2957 M0III SB1 Arc 14 9 −1.41 1.49 0.17 (38) R CORAVEL −0.23 ± 0.15
111170 1479 F7V nRV<10 SB2 G2 6,6 139,28 0.66,0.70 4.22,7.47 1.11,2.93 (3) R CORAVEL +0.32 ± 0.10
115126 1438 G5IV+K2V SB1 Arc 2 27 0.56 0.07 0.02 (29) R HIDES +0.65 ± 0.08
115142A 2860 F3IV−V nRV<10 SB2 F0ROT 4,4 64 −3.30,10.93 8.72,21.75 1.35 (39) R CamCOR +0.20 ± 0.10
115142B (i) 2859 M3V nRV<10 SB1 F0 6 25 −1.31 3.78 1.44 (40) R Simeis +0.29 ± 0.54

Notes. See Sect. 2 for details about the content of each column. (a)The orbit listed in Table 4 is computed from HERMES RVs only. (b)Based on lines from the cool component. (c)It is unclear whether that spectral combination corresponds to the pair AB or Aa,Ab (see text). (d)The violet Balmer lines from the hot component are too wide to derive a precise RV from the HERMES spectra. (e)Composite nature of this spectrum not confirmed by HERMES (see Sect. A). (f)Component spectral type derived from 0.6 M⊙ mass from Anguita-Aguero et al. (2022). (g)Not seen as SB2 by HERMES. (h)See HIP 91751 in Appendix A. (i)Although HIP 115142B is not an entry of the SIMBAD database, it is used here for convenience. Use HD 219877B in SIMBAD instead.

References. (1) González & Levato (2009); (2) Harper (1926); (3) Pourbaix (2000); (4) Griffin (1980); (5) Halbwachs et al. (2016); (6) De Cat et al. (2000); (7) Popper (1988); (8) Abt (1965); (9) Griffin (2006); (10) Welty & Wade (1995); (11) Udry et al. (1998b); (12) Mermilliod et al. (2007); (13) Griffin (2005); (14) Carquillat et al. (2003); (15) Wade et al. (1999); (16) Carquillat & Prieur (2008); (17) Udry et al. (1998a); (18) Massarotti et al. (2008); (19) Carquillat & Prieur (2007); (20) Griffin (2004); (21) Carney et al. (2001); (22) Spencer Jones (1928); (23) Torres (2006); (24) Torres et al. (1995); (25) Griffin (2010); (26) Hockey (1969); (27) Zhao et al. (2007); (28) Forveille et al. (1999); (29) Katoh et al. (2013); (30) Duquennoy et al. (1992); (31) Radford & Griffin (1977); (32) Stockton & Fekel (1992); (33) Smekhov (2002); (34) Franklin (1952); (35) Seydel (1931); (36) Willmarth et al. (2016); (37) McClure (1997); (38) Famaey et al. (2009); (39) Griffin (2009); (40) Griffin (2009).

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